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Evolutionary processes in binary and multiple stars /

Binary systems of stars are as common as single stars. Stars evolve primarily by nuclear reactions in their interiors, but a star with a binary companion can also have its evolution influenced by the companion. Multiple star systems can exist stably for millions of years, but can ultimately become u...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor principal: Eggleton, P. P. (Peter P.), 1940-
Formato: Electrónico eBook
Idioma:Inglés
Publicado: Cambridge, UK ; New York : Cambridge University Press, 2006.
Colección:Cambridge astrophysics series ; 40.
Temas:
Acceso en línea:Texto completo
Tabla de Contenidos:
  • Cover; Half-title; Series-title; Title; Copyright; Contents; Preface; 1 Introduction; 2 Evolution of single stars; 3 Binary interaction: conservative processes; 4 Slow non-conservative processes; 5 Rapid non-conservative processes; 6 Accretion by the companion; Appendix A The equations of stellar structure; Appendix B Distortion and circulation in a non-spherical star; Appendix C Perturbations to Keplerian orbits; Appendix D Steady, axisymmetric magnetic winds; Appendix E Stellar dynamos; Appendix F Steady, axisymmetric, cool accretion discs; References; Subject index; Stellar objects index